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New Optical and Infrared Photometric Study of Young Open Star Cluster NGC 7790

机译:新的光学和红外线光度研究NGC 7790

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摘要

We present deep CCD photometry (V similar to 21 mag) in BVR Johnson-Cousin filters supported with 2MASS JHKs data set for the open star cluster NGC 7790. The cluster's parameters such as reddening, distance, metallicity and age etc horizontal ellipsis are derived using two color diagrams in optical and near-infrared bands. These parameters areE(B-V)= 0.512 +/- 0.006,EV-R= 0.382 +/- 0.005,EJ-H= 0.337 +/- 0.001 andE(J-Ks)= 0.505 +/- 0.001 mag, the distance modulus (m-M)(0)= 12.41 +/- 0.001 mag, which gives a distance of 3.035 kpc and the metallicityZ= 0.008. The age obtained by fitting the observed CMDs with Padova isochrones is 63.95 Myr. From the analysis of 2MASS data, the limiting radius of the cluster is found to be 9.7 +/- 0.83 arcmin, it reflects that the cluster is a compact cluster. The dynamical relaxation time of NGC 7790 is also determined and found to be 0.17 of its age, which means that the cluster is dynamically relaxed. Moreover, luminosity and mass functions are also investigated.
机译:我们在BVR Johnson-Cousin滤波器中呈现深度CCD光度测量(V类似于21 Mag),该jhks-cousin滤波器为Open Star Cluster NGC 7790支持。群集的参数,例如ReDdening,距离,金属性和年龄级别省略水平省略量光学和近红外频段的两种颜色图。这些参数AREE(BV)= 0.512 +/- 0.006,EV-R = 0.382 +/- 0.005,EJ-H = 0.337 +/- 0.001和E(J-KS)= 0.505 +/- 0.001 mag,距离模量( mm)(0)= 12.41 +/- 0.001 mag,其距离为3.035 kpc,金属性= 0.008。通过与Padova同种影酮拟合观察到的CMDS获得的年龄是63.95 MYR。从分析2MASS数据,发现群集的限制半径为9.7 +/- 0.83 arcmin,它反映了群集是一个紧凑的群集。 NGC 7790的动态松弛时间也被确定并发现其年龄的0.17,这意味着簇被动态地松弛。此外,还研究了亮度和质量功能。

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